Fe-Ni-S-O layer phase in C2M carbonaceous chondrites - A hydrous sulphide?

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Carbonaceous Chondrites, Hydrogen Sulfide, Meteoritic Composition, Diffraction Patterns, Electron Microscopy, Energy Spectra, Lattice Parameters, Troilite, Meteorites, Carbonaceous Chondrites, Phases, C2M Chondrites, Sulfides, Iron, Nickel, Mineralogy, Sulfur, Oxygen, Matrix, Formation, Hvhrem, Hydration, Comparisons, Morphology, Electron Microscopy, Spectrometry, X-Rays, Electrons, Murchison, Cold Bokkeveld, Nawapali, Spectra, Photomicrographs, Data

Scientific paper

Poorly-characterized phases (PCP) containing Fe, Ni, S, O and sometimes Cr, were first noted in the matrix material of the Murchison meteorite. Barber found that amongst PCP there was a layer phase, rich in Fe, Ni, S and thought to contain oxygen, commonly having a fibrous or platey morphology. The authors report new data on this phase, obtained by high resolution electron microscopy, dispersive X-ray spectrometry and electron energy loss spectrometry, and they conclude that it is probably a hydrous sulphide.

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